Abstract

The vacuum energy density now is small or zero but must have been prodigious if the universe was once hotter than ${T}_{c}\ensuremath{\sim}{10}^{15}$ K and if elementary-particle symmetry is spontaneously broken by a Higgs mechanism. If symmetry is broken nondynamically, in the hot disordered phase the huge vacuum energy density is nevertheless negligible, compared to the energy density of ultrarelativistic particles. Because the broken symmetry is non-Abelian, the long-range forces arising on symmetry restoration need not lead back to an anisotropic, inhomogeneous, or domain-structure universe.

Keywords

PhysicsVacuum energySymmetry (geometry)Cosmological constantSymmetry breakingHiggs bosonPhase transitionUniverseSpontaneous symmetry breakingFalse vacuumDiscrete symmetryCondensed matter physicsTheoretical physicsQuantum mechanicsGeometryHomogeneous space

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Publication Info

Year
1977
Type
article
Volume
38
Issue
5
Pages
255-257
Citations
102
Access
Closed

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S. A. Bludman, M. Ruderman (1977). Induced Cosmological Constant Expected above the Phase Transition Restoring the Broken Symmetry. Physical Review Letters , 38 (5) , 255-257. https://doi.org/10.1103/physrevlett.38.255

Identifiers

DOI
10.1103/physrevlett.38.255